Since, the initial velocity of body is zero, its total energy is E=r−GmM ...(i)
where, m is the mass of body, M is the mass of the Earth and r its distance from the centre of the Earth. When the body reaches the Earth, let its, velocity be v and its distance from the centre of the Earth equals the Earths radius R. Therefore, the energy is E=21mv2−RGMm ...(ii)
Equating Eqs. (i) and (ii), we get v2=2GM(R1−r1)
Also, g=R2GM. Therefore, GM=gR2.
Using this in the above equation, we get V=R[2g(R1−r1)]1/2
Now, r=2R (given). Therefore, V=R[2g(R1−2R1)]1/2 ⇒ Velocity of a body which strike the Earth's surface, v=gR